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Time Evolution in Dynamical Spacetimes

A. Tiemblo·R. Tresguerres
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Abstract

We present a gauge--theoretical derivation of the notion of time, suitable to describe the Hamiltonian time evolution of gravitational systems. It is based on a nonlinear coset realization of the Poincaré group, implying the time component of the coframe to be invariant, and thus to represent a metric time. The unitary gauge fixing of the boosts gives rise to the foliation of spacetime along the time direction. The three supressed degrees of freedom correspond to Goldstone--like fields, whereas the remaining time component is a Higgs--like boson.

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A. Tiemblo, R. Tresguerres. 1996-07-26. Time Evolution in Dynamical Spacetimes. https://arxiv.org/abs/gr-qc/9607066

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